XSvsedov¶
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class
sherpa.astro.xspec.
XSvsedov
(name='vsedov')[source] [edit on github]¶ Bases:
sherpa.astro.xspec.XSAdditiveModel
The XSPEC vsedov model: sedov model, separate ion/electron temperature.
The model is described at 1. The
set_xsxset
andget_xsxset
functions are used to set and query the XSPEC XSET parameters, in particular the keyword “NEIVERS”.-
kT_a
¶ The mean shock temperature, in keV.
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kT_b
¶ The electron temperature immediately behind the shock front, in keV. See 1 for a discussion of the behavior of kT_a and kT_b.
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H
¶ The H abundance: it should be set to 0 to switch on and 1 to switch off the free-free continuum.
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He, C, N, O, Ne, Mg, Si, S, Ar, Ca, Fe, Ni
The abundance of the element, with respect to Solar.
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Tau
¶ The ionization timescale in units of s/cm^3.
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redshift
¶ The redshift of the plasma.
References
Attributes Summary
The hard maximum values for the thawed parameters.
The hard minimum values for the thawed parameters.
Access to the maximum limits for the thawed parameters
Access to the minimum limits for the thawed parameters
Access to the thawed parameters of the model
Methods Summary
apply
(outer, *otherargs, **otherkwargs)calc
(pars, xlo, *args, **kwargs)Evaluate the model on a grid.
guess
(dep, *args, **kwargs)Set an initial guess for the parameter values.
regrid
(*args, **kwargs)The class RegriddableModel1D allows the user to evaluate in the requested space then interpolate onto the data space.
reset
()Reset the parameter values.
set_center
(*args, **kwargs)startup
([cache])Called before a model may be evaluated multiple times.
teardown
()Called after a model may be evaluated multiple times.
Attributes Documentation
-
ndim
= 1¶
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thawedparhardmaxes
¶ The hard maximum values for the thawed parameters.
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thawedparhardmins
¶ The hard minimum values for the thawed parameters.
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thawedparmaxes
¶ Access to the maximum limits for the thawed parameters
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thawedparmins
¶ Access to the minimum limits for the thawed parameters
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thawedpars
¶ Access to the thawed parameters of the model
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version_enabled
= True¶
Methods Documentation
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apply
(outer, *otherargs, **otherkwargs) [edit on github]¶
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calc
(pars, xlo, *args, **kwargs) [edit on github]¶ Evaluate the model on a grid.
- Parameters
p (sequence of numbers) – The parameter values to use. The order matches the
pars
field.*args – The model grid. The values can be scalar or arrays, and the number depends on the dimensionality of the model and whether it is being evaluated over an integrated grid or at a point (or points).
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get_center
() [edit on github]¶
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guess
(dep, *args, **kwargs) [edit on github]¶ Set an initial guess for the parameter values.
Attempt to set the parameter values, and ranges, for the model to match the data values. This is intended as a rough guess, so it is expected that the model is only evaluated a small number of times, if at all.
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regrid
(*args, **kwargs) [edit on github]¶ The class RegriddableModel1D allows the user to evaluate in the requested space then interpolate onto the data space. An optional argument ‘interp’ enables the user to change the interpolation method.
Examples
>>> import numpy as np >>> from sherpa.models.basic import Box1D >>> mybox = Box1D() >>> request_space = np.arange(1, 10, 0.1) >>> regrid_model = mybox.regrid(request_space, interp=linear_interp)
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reset
() [edit on github]¶ Reset the parameter values.
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set_center
(*args, **kwargs) [edit on github]¶
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startup
(cache=False) [edit on github]¶ Called before a model may be evaluated multiple times.
- Parameters
cache (bool, optional) – Should a cache be used when evaluating the models.
See also
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teardown
() [edit on github]¶ Called after a model may be evaluated multiple times.
See also
setup()
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